Applications are invited for two Postdoctoral Research Assistant positions in Warm Dense Matter (Theory/Computation/Experiments).

 

The post is available initially for a fixed-term duration of   2.5  years.

 

Exotic and high-pressure warm dense matter (WDM) states exists in gas giants, brown and white dwarf stars, the crust of neutron stars, and it can be created during Inertial Confinement Fusion (ICF) experiments. Warm dense matter is a strongly coupled quantum plasma, with ions moving in a partially degenerate electron fluid, and having kinetic energy comparable to the ion-ion interaction energy. Consequently, WDM inherits properties from both condensed matter systems and classical plasmas. Measuring a modelling the equation of state as well as other thermodynamic and transport properties of WDM is crucial not only for our understanding of astrophysical objects but also for the success of ICF.

We are looking for two postdocs in WDM studies. One vacancy is for an experimental scientist, to measure heat transport  and viscosity in WDM systems under different drive conditions. For the other vacancy we  are looking for a theory/computational scientist to perform large scale simulations of WDM plasmas using quantum simulation techniques based on Molecular Dynamics and/or Density Functional Theory.

 

For the experimental position, we expect the successful candidate to be involved in the planning, execution and analysis of experiments at high power laser facilities and fourth generation light sources. For the theory/computational position, we intend the ideal candidate to perform high-performance computing modelling of transport in WDM and compare predictions against experimental data. For both positions, we expect Machine Learning techniques to be used/deployed in the data analysis and in the creation of surrogate models.

 

The post-holder will have the opportunity to teach. This may include lecturing, small group teaching, and tutoring of undergraduates and graduate students.

 

Applicants should hold a PhD, or be close to completion in physics or a related field and have a strong background in plasma physics.

 

Previous experience (theory/experiments) in planetary physics and/or ICF research is welcome.

 

Candidates are expected to be able to work in a multidisciplinary environment.

 

Please direct enquiries about the role to Prof Gianluca Gregori and Prof Sam Vinko. (gianluca.gregori@physics.ox.ac.uk) (sam.vinko@physics.ox.ac.uk)

 

Only applications received before midday (UK time) 9 June 2023 can be considered. You will be required to upload a statement of research interests, CV and details of two referees as part of your online application.